lbw sefd curves after New lbw feed installed.

Mar03-Jun06

Links to the plots:
the sefd fits vs za with the fit residuals (.ps). (.pdf)
fits using za and az terms (for comparison)  (.pdf)

    The lband wide receiver was replaced in feb03.  All of the lbw calibration scans between mar03 and jun06 were used to fit curves to the SEFD.  Frequency data was taken at: :(1175,1300,1375,1415) and (1415,1550,1610,1666). sefd curves were then computed fitting for sefd as a function of za (fits using azimuth terms did not improve the fit enough to make a difference).  The fitting function (with za in degrees) is:

g(za)=c0 +c1*za + c2*(za-14)^2 +c3*(za-14)^3
where the ^2 and ^3 terms are only applied for za ge 14 degrees.
There were a total of 8373 measurements over all frequencies.

The plots show  the sefd fits vs za with the fit residuals (.ps). (.pdf) :

Summary of sefd fits
freq # of points fit rms
Jy
1175
1260
.18
1300
1260
.15
1375
1256
.15
1415
2096
.14
1550
832
.15
1610
833
.16
1665
836
.15

      1415 Mhz has twice the measurements for the fits since it was included in both frequency groups. The sefd decreases from 1175 to 1415 Mhz and then remains relatively constant. Most of this is probably coming from Tsys decreasing as we move to higher frequency.

Note: The fits using za and az terms  (.pdf) are available for comparison. They are not the curves being used.


  The idl routines sefdget() or corhsefdget() will now return the lbw sefd for data after 01mar03 using these fits. The coefficients can be found in the ascii file  data/sefd.datR5 (this is provided in the AO idl distribution for correlator routines). You can also find a copy of it at AO in /home/phil/idl/data/sefd.datR5.
processing: x101/lb/Mar03/dosefdfit.pro

 

 

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